collaborators

6 papers

astro-ph.SR2025

Characterizing Vortex-Driven Dynamics in the Solar Atmosphere Using Information Theory

Suzana S. A. Silva, Erico Rempel, Gary Verth +2

Solar vortex regions show enhanced Poynting flux and favourable heating conditions, but how the vortices reorganize and influence their surroundings remains unclear. Here we apply…

astro-ph.SR2025

Alfven Waves in Partially Ionised Solar Steady-State Plasmas

Nada F. Alshehri, Istvan Ballai, Viktor Fedun +1

Our study investigates the properties of Alfvén waves in partially ionised solar plasmas in the presence of steady, field-aligned, flows of charged and neutral particles. Our work…

astro-ph.SR2025

Solar Vortices as Conduits for Magnetoacoustic Waves: Multi-Layer Coupling and Their Role in Atmospheric Heating

Suzana S. A. Silva, Ioannis Dakanalis, Luiz A. C. A. Schiavo +10

The Sun's atmosphere hosts swirling plasma structures, known as solar vortices, which have long been thought to channel wave energy into higher layers. Until now, no direct observa…

astro-ph.SR2025

Global CME-driven oscillations in the outer solar corona

Suzana S. A. Silva, J. J. Gonzalez-Aviles, Pete Riley +8

Coronal mass ejections (CMEs) are known drivers of large-scale waves in the low corona. However, wave dynamics in the extended corona and inner heliosphere remain largely unexplore…

astro-ph.SR2025

Driven phase-mixed Alfvén waves in a partially ionized solar plasma

Max McMurdo, Istvan Ballai, Gary Verth +1

Phase mixing has long been understood to be a viable mechanism for expediting the dissipation of Alfvén wave energy resulting in the subsequent heating of the solar atmosphere. To…

astro-ph.SR2025

3D MHD wave propagation and energy transport in a simulated solar vortex

Samuel Skirvin, Viktor Fedun, Gary Verth +1

Magnetic flux tubes in the presence of background rotational flows are abundant throughout the solar atmosphere and may act as conduits for MHD waves to transport energy throughout…